Английская Википедия:Dynamical horizon

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Версия от 01:09, 1 марта 2024; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} {{primary sources|date=March 2012}} In theoretical physics, a '''dynamical horizon''' (DH) is a local description (i.e. independent of the global structure of space–time) of evolving black-hole horizons. In the literature there exist two different mathematical formulations of DHs—the 2+2 formulation developed first by Sean Hayward and the 3+1 formulation developed by ...»)
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Шаблон:Primary sources In theoretical physics, a dynamical horizon (DH) is a local description (i.e. independent of the global structure of space–time) of evolving black-hole horizons. In the literature there exist two different mathematical formulations of DHs—the 2+2 formulation developed first by Sean Hayward and the 3+1 formulation developed by Abhay Ashtekar and others (see Шаблон:Harvnb).Шаблон:Sfn It provides a description of a black hole that is evolving (e.g. one that has a non-zero mass–energy influx).Шаблон:Sfn A related formalism, for black holes with zero influx, is an isolated horizon.

Formal definition

The formal definition of a dynamical horizon is as follows: Шаблон:Quote

See also

References

Cross-reference

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Sources used

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Further reading

Broad outlines

Major papers

Other work


Шаблон:Relativity-stub

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